As soluções de buracos negros: 1916-1965

Autores

DOI:

https://doi.org/10.47456/Cad.Astro.v4n1.39861

Palavras-chave:

estrelas invisíveis, buracos negros, Schwarzschild, Reissner-Nordström, Kerr, Newman, extensões analíticas, massas pontuais

Resumo

Historicamente, as primeiras soluções da relatividade geral não foram reconhecidas como soluções de buracos negros. Elas foram, a princípio, idealizadas para descrever o campo gravitacional de objetos massivos esfericamente simétricos, como o Sol ou o elétron. Neste artigo, vamos apresentar as soluções de buracos negros em seu contexto histórico e mostrar como a nossa compreensão sobre o universo mudou à medida que desvendamos propriedades fundamentais sobre estes campos gravitacionais. O objetivo é apresentar uma introdução histórica sobre a relatividade geral e buracos negros, focada na teoria de gravitação e suas interpretações, como apoio didático para aqueles que pretendem iniciar os estudos sobre o tema.

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Publicado

10-03-2023

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[1]
C. R. Almeida, “As soluções de buracos negros: 1916-1965”, Cad. Astro., vol. 4, nº 1, p. 16–34, mar. 2023.

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